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Statements

Subject Item
dbr:Index_of_physics_articles_(C)
dbo:wikiPageWikiLink
dbr:CORSIKA
Subject Item
dbr:UrQMD
dbo:wikiPageWikiLink
dbr:CORSIKA
Subject Item
dbr:Air_shower_(physics)
dbo:wikiPageWikiLink
dbr:CORSIKA
Subject Item
dbr:KASCADE
dbo:wikiPageWikiLink
dbr:CORSIKA
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rdfs:label
CORSIKA
rdfs:comment
CORSIKA (COsmic Ray SImulations for KAscade) is a physics computer software for simulation of extensive air showers induced by high energy cosmic rays, i.e. protons and atomic nuclei, as well as Gamma rays (photons), electrons, and neutrinos. It may be used up to and beyond the highest energies of 100 EeV. It can be used to simulate the generation of Cherenkov radiation, radio emission (Askaryan radiation), and atmospheric neutrinos. A complete rewrite of CORSIKA in C++ named CORSIKA 8 is currently work in progress.
foaf:name
CORSIKA, an Extensive Air Shower Simulation Program
foaf:homepage
n12:
dbp:name
an Extensive Air Shower Simulation Program CORSIKA,
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n5:abstract%3Fid=oai%3AarXiv.org%3Aastro-ph%2F0103073 n12: n17:icrc_durban.pdf n19:gap_2001_059.ps n25:technicalities.html
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dbr:Tanguy_Pierog dbr:Institut_für_Astroteilchenphysik dbr:Johannes_Knapp dbr:Zeuthen dbr:Forschungszentrum_Karlsruhe dbr:Dieter_Heck dbr:Deutsches_Elektronen-Synchrotron dbr:Germany
dbp:developer
CORSIKA collaboration
dbp:genre
dbr:Astroparticle_physics
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dbp:latestReleaseDate
2021-05-01
dbp:latestReleaseVersion
7.741
dbp:license
CORSIKA is available to every scientist free of charge (more)
dbp:website
n12:
dbo:abstract
CORSIKA (COsmic Ray SImulations for KAscade) is a physics computer software for simulation of extensive air showers induced by high energy cosmic rays, i.e. protons and atomic nuclei, as well as Gamma rays (photons), electrons, and neutrinos. It may be used up to and beyond the highest energies of 100 EeV. In the current version the program utilizes the hadronic interaction models EPOS, , and , which are based on , and based on a model for highenergies. Hadronic interactions at lower energies are described either by the module, by FLUKA, or by the UrQMD model. Electromagnetic interactions are treated by an adapted version of the EGS4 code,customized by including the Landau–Pomeranchuk–Migdal effect relevant at higher energies. It can be used to simulate the generation of Cherenkov radiation, radio emission (Askaryan radiation), and atmospheric neutrinos. A complete rewrite of CORSIKA in C++ named CORSIKA 8 is currently work in progress.
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dbr:Astroparticle_physics
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dbr:FORTRAN_77
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dbr:Free_of_charge
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wikipedia-en:CORSIKA
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